ORCS Documentation¶
Contents
Features¶
ORCS (Outils de Réduction de Cubes Spectraux) is an analysis engine for SITELLE spectral cubes. With ORCS you can:
extract integrated spectra
fit the sinc emission lines
recalibrate your data in wavelength, astrometry and flux
choose between a Bayesian or a classical fitting algorithm
and much more …
Examples in Jupyter format can be found in Examples.
Warning
ORCS is always in fast development. You might see bugs or strange behaviours ! You might also want desperatly to have new features. In all cases please send an email: thomas.martin.1@ulaval.ca
Publications¶
Martin, Drissen, Melchior (2017). A SITELLE view of M31’s central region - I: Calibrations and radial velocity catalogue of nearly 800 emission-line point-like sources. MNRAS (accepted) http://adsabs.harvard.edu/abs/2017arXiv170701366M
Martin, Drissen (2017). SITELLE’s level-1 calibration. MNRAS (submitted) http://adsabs.harvard.edu/abs/2017arXiv170603230M
Martin, Prunet, Drissen (2016). Optimal fitting of Gaussian-apodized or under-resolved emission lines in Fourier transform spectra providing new insights on the velocity structure of NGC 6720. MNRAS http://adsabs.harvard.edu/abs/2016MNRAS.463.4223M
Martin, Drissen, Joncas (2015). ORBS, ORCS, OACS, a Software Suite for Data Reduction and Analysis of the Hyperspectral Imagers SITELLE and SpIOMM. PASP http://adsabs.harvard.edu/abs/2015ASPC..495..327M